Non-Gaussianity and CMB aberration and Doppler

Abstract

The peculiar motion of an observer with respect to the CMB rest frame induces a deflection in the arrival direction of the observed photons (also known as CMB aberration) and a Doppler shift in the measured photon frequencies. As a consequence, aberration and Doppler effects induce non trivial correlations between the harmonic coefficients of the observed CMB temperature maps. In this paper we investigate whether these correlations generate a bias on Non-Gaussianity estimators $f_{NL}$. We perform this analysis simulating a large number of temperature maps with Planck-like resolution (lmax $=2000$) as different realizations of the same cosmological fiducial model (WMAP7yr). We then add to these maps aberration and Doppler effects employing a modified version of the HEALPix code. We finally evaluate a generalization of the Komatsu, Spergel and Wandelt Non-Gaussianity estimator for all the simulated maps, both when peculiar velocity effects have been considered and when these phenomena have been neglected. Using the value $v/c=1.23\times 10^{-3}$ for our peculiar velocity, we found that the aberration/Doppler induced Non-Gaussian signal is at most of about half of the cosmic variance $\sigma$ for $f_{NL}$ both in a full-sky and in a cut-sky experimental configuration, for local, equilateral and orthogonal estimators. We conclude therefore that when estimating $f_{NL}$ it is safe to ignore aberration and Doppler effects {\it if} the primordial map is already Gaussian. More work is necessary however to assess whether a map which contains Non-Gaussianity can be significantly distorted by a peculiar velocity.

13 pages, 6 figures

References in corpus (3)

• The Signature of Proper Motion in the Microwave Sky
• Real Space Approach to CMB deboosting
• Effects of a Cut, Lorentz-Boosted sky on the Angular Power Spectrum

Cited by in corpus (5)

• Planck 2013 results. XXVII. Doppler boosting of the CMB: Eppur si muove
• On the significance of power asymmetries in Planck CMB data at all scales
• Disentangling Doppler modulation, aberration and the temperature dipole in the CMB
• A Generalized Doppler and Aberration Kernel for Frequency-Dependent Cosmological Observables
• Effects of boosting on extragalactic components: methods and statistical studies